Black holes in Einstein–Gauss–Bonnet gravity with a string cloud background
- Autores
- Herscovich Ramoneda, Estanislao Benito; Richarte, Martín Gustavo
- Año de publicación
- 2010
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We obtain a black hole solution in the Einstein–Gauss–Bonnet theory for the string cloud model in a five-dimensional spacetime. We analyze the event horizons and naked singularities. Later, we compute the Hawking temperature TH, the specific heat C, the entropy S, and the Helmholtz free energy F of the black hole. The entropy was computed using the Wald formulation. In addition, the quantum correction to the Wald's entropy is considered for the string cloud source. We mainly explore the thermodynamical global and local stability of the system with vanishing or non-vanishing cosmological constant. The global thermodynamic phase structure indicates that the Hawking–Page transition is achieved for this model. Further, we observe that there exist stable black holes with small radii and that these regions are enlarged when choosing small values of the string cloud density and of the Gauss–Bonnet parameter. Besides, the rate of evaporation for these black holes are studied, determining whether the evaporation time is finite or not. Then, we concentrate on the dynamical stability of the system, studying the effective potential for s-waves propagating on the string cloud background.
Fil: Herscovich Ramoneda, Estanislao Benito. Universität Paderborn; Alemania. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Richarte, Martín Gustavo. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina - Materia
-
Einstein-Gauss-Bonnet gravity
String cloud model
Black Holes
5-dimension - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-nd/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/16395
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Black holes in Einstein–Gauss–Bonnet gravity with a string cloud backgroundHerscovich Ramoneda, Estanislao BenitoRicharte, Martín GustavoEinstein-Gauss-Bonnet gravityString cloud modelBlack Holes5-dimensionhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We obtain a black hole solution in the Einstein–Gauss–Bonnet theory for the string cloud model in a five-dimensional spacetime. We analyze the event horizons and naked singularities. Later, we compute the Hawking temperature TH, the specific heat C, the entropy S, and the Helmholtz free energy F of the black hole. The entropy was computed using the Wald formulation. In addition, the quantum correction to the Wald's entropy is considered for the string cloud source. We mainly explore the thermodynamical global and local stability of the system with vanishing or non-vanishing cosmological constant. The global thermodynamic phase structure indicates that the Hawking–Page transition is achieved for this model. Further, we observe that there exist stable black holes with small radii and that these regions are enlarged when choosing small values of the string cloud density and of the Gauss–Bonnet parameter. Besides, the rate of evaporation for these black holes are studied, determining whether the evaporation time is finite or not. Then, we concentrate on the dynamical stability of the system, studying the effective potential for s-waves propagating on the string cloud background.Fil: Herscovich Ramoneda, Estanislao Benito. Universität Paderborn; Alemania. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Richarte, Martín Gustavo. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaElsevier Science2010-05info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/16395Herscovich Ramoneda, Estanislao Benito; Richarte, Martín Gustavo; Black holes in Einstein–Gauss–Bonnet gravity with a string cloud background; Elsevier Science; Physics Letters B; 689; 4-5; 5-2010; 192-2000370-2693enginfo:eu-repo/semantics/altIdentifier/doi/10.1016/j.physletb.2010.04.065info:eu-repo/semantics/altIdentifier/url/http://www.sciencedirect.com/science/article/pii/S0370269310005514info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-nd/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:01:50Zoai:ri.conicet.gov.ar:11336/16395instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:01:51.238CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Black holes in Einstein–Gauss–Bonnet gravity with a string cloud background |
title |
Black holes in Einstein–Gauss–Bonnet gravity with a string cloud background |
spellingShingle |
Black holes in Einstein–Gauss–Bonnet gravity with a string cloud background Herscovich Ramoneda, Estanislao Benito Einstein-Gauss-Bonnet gravity String cloud model Black Holes 5-dimension |
title_short |
Black holes in Einstein–Gauss–Bonnet gravity with a string cloud background |
title_full |
Black holes in Einstein–Gauss–Bonnet gravity with a string cloud background |
title_fullStr |
Black holes in Einstein–Gauss–Bonnet gravity with a string cloud background |
title_full_unstemmed |
Black holes in Einstein–Gauss–Bonnet gravity with a string cloud background |
title_sort |
Black holes in Einstein–Gauss–Bonnet gravity with a string cloud background |
dc.creator.none.fl_str_mv |
Herscovich Ramoneda, Estanislao Benito Richarte, Martín Gustavo |
author |
Herscovich Ramoneda, Estanislao Benito |
author_facet |
Herscovich Ramoneda, Estanislao Benito Richarte, Martín Gustavo |
author_role |
author |
author2 |
Richarte, Martín Gustavo |
author2_role |
author |
dc.subject.none.fl_str_mv |
Einstein-Gauss-Bonnet gravity String cloud model Black Holes 5-dimension |
topic |
Einstein-Gauss-Bonnet gravity String cloud model Black Holes 5-dimension |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We obtain a black hole solution in the Einstein–Gauss–Bonnet theory for the string cloud model in a five-dimensional spacetime. We analyze the event horizons and naked singularities. Later, we compute the Hawking temperature TH, the specific heat C, the entropy S, and the Helmholtz free energy F of the black hole. The entropy was computed using the Wald formulation. In addition, the quantum correction to the Wald's entropy is considered for the string cloud source. We mainly explore the thermodynamical global and local stability of the system with vanishing or non-vanishing cosmological constant. The global thermodynamic phase structure indicates that the Hawking–Page transition is achieved for this model. Further, we observe that there exist stable black holes with small radii and that these regions are enlarged when choosing small values of the string cloud density and of the Gauss–Bonnet parameter. Besides, the rate of evaporation for these black holes are studied, determining whether the evaporation time is finite or not. Then, we concentrate on the dynamical stability of the system, studying the effective potential for s-waves propagating on the string cloud background. Fil: Herscovich Ramoneda, Estanislao Benito. Universität Paderborn; Alemania. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Richarte, Martín Gustavo. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina |
description |
We obtain a black hole solution in the Einstein–Gauss–Bonnet theory for the string cloud model in a five-dimensional spacetime. We analyze the event horizons and naked singularities. Later, we compute the Hawking temperature TH, the specific heat C, the entropy S, and the Helmholtz free energy F of the black hole. The entropy was computed using the Wald formulation. In addition, the quantum correction to the Wald's entropy is considered for the string cloud source. We mainly explore the thermodynamical global and local stability of the system with vanishing or non-vanishing cosmological constant. The global thermodynamic phase structure indicates that the Hawking–Page transition is achieved for this model. Further, we observe that there exist stable black holes with small radii and that these regions are enlarged when choosing small values of the string cloud density and of the Gauss–Bonnet parameter. Besides, the rate of evaporation for these black holes are studied, determining whether the evaporation time is finite or not. Then, we concentrate on the dynamical stability of the system, studying the effective potential for s-waves propagating on the string cloud background. |
publishDate |
2010 |
dc.date.none.fl_str_mv |
2010-05 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/16395 Herscovich Ramoneda, Estanislao Benito; Richarte, Martín Gustavo; Black holes in Einstein–Gauss–Bonnet gravity with a string cloud background; Elsevier Science; Physics Letters B; 689; 4-5; 5-2010; 192-200 0370-2693 |
url |
http://hdl.handle.net/11336/16395 |
identifier_str_mv |
Herscovich Ramoneda, Estanislao Benito; Richarte, Martín Gustavo; Black holes in Einstein–Gauss–Bonnet gravity with a string cloud background; Elsevier Science; Physics Letters B; 689; 4-5; 5-2010; 192-200 0370-2693 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1016/j.physletb.2010.04.065 info:eu-repo/semantics/altIdentifier/url/http://www.sciencedirect.com/science/article/pii/S0370269310005514 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-nd/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-nd/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Elsevier Science |
publisher.none.fl_str_mv |
Elsevier Science |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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13.070432 |